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@article{Aghanim:2020:0004-6361/201833880,
author = {Aghanim, N and Akrami, Y and Arroja, F and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, AJ and Barreiro, RB and Bartolo, N and Basak, S and Battye, R and Benabed, K and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bock, JJ and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Cardoso, J-F and Carron, J and Casaponsa, B and Challinor, A and Chiang, HC and Colombo, LPL and Combet, C and Contreras, D and Crill, BP and Cuttaia, F and de, Bernardis P and de, Zotti G and Delabrouille, J and Delouis, J-M and Desert, F-X and Di, Valentino E and Dickinson, C and Diego, JM and Donzelli, S and Dore, O and Douspis, M and Ducout, A and Dupac, X and Efstathiou, G and Elsner, F and Ensslin, TA and Eriksen, HK and Falgarone, E and Fantaye, Y and Fergusson, J and Fernandez-Cobos, R and Finelli, F and Forastieri, F and Frailis, M and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ga},
doi = {0004-6361/201833880},
journal = {Astronomy and Astrophysics: a European journal},
title = {Planck 2018 results: I. Overview and the cosmological legacy of Planck},
url = {http://dx.doi.org/10.1051/0004-6361/201833880},
volume = {641},
year = {2020}
}

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TY  - JOUR
AB  - The European Space Agency’s Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. This paper presents the cosmological legacy of Planck, which currently provides our strongest constraints on the parameters of the standard cosmological model and some of the tightest limits available on deviations from that model. The 6-parameter ΛCDM model continues to provide an excellent fit to the cosmic microwave background data at high and low redshift, describing the cosmological information in over a billion map pixels with just six parameters. With 18 peaks in the temperature and polarization angular power spectra constrained well, Planck measures five of the six parameters to better than 1% (simultaneously), with the best-determined parameter (θ) now known to 0.03%. We describe the multi-component sky as seen by Planck, the success of the ΛCDM model, and the connection to lower-redshift probes of structure formation. We also give a comprehensive summary of the major changes introduced in this 2018 release. The Planck data, alone and in combination with other probes, provide stringent constraints on our models of the early Universe and the large-scale structure within which all astrophysical objects form and evolve. We discuss some lessons learned from the Planck mission, and highlight areas ripe for further experimental advances.
AU  - Aghanim,N
AU  - Akrami,Y
AU  - Arroja,F
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Ballardini,M
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartolo,N
AU  - Basak,S
AU  - Battye,R
AU  - Benabed,K
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bock,JJ
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Boulanger,F
AU  - Bucher,M
AU  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Cardoso,J-F
AU  - Carron,J
AU  - Casaponsa,B
AU  - Challinor,A
AU  - Chiang,HC
AU  - Colombo,LPL
AU  - Combet,C
AU  - Contreras,D
AU  - Crill,BP
AU  - Cuttaia,F
AU  - de,Bernardis P
AU  - de,Zotti G
AU  - Delabrouille,J
AU  - Delouis,J-M
AU  - Desert,F-X
AU  - Di,Valentino E
AU  - Dickinson,C
AU  - Diego,JM
AU  - Donzelli,S
AU  - Dore,O
AU  - Douspis,M
AU  - Ducout,A
AU  - Dupac,X
AU  - Efstathiou,G
AU  - Elsner,F
AU  - Ensslin,TA
AU  - Eriksen,HK
AU  - Falgarone,E
AU  - Fantaye,Y
AU  - Fergusson,J
AU  - Fernandez-Cobos,R
AU  - Finelli,F
AU  - Forastieri,F
AU  - Frailis,M
AU  - Franceschi,E
AU  - Frolov,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Genova-Santos,RT
AU  - Gerbino,M
AU  - Ghosh,T
AU  - Gonzalez-Nuevo,J
AU  - Gorski,KM
AU  - Gratton,S
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Hamann,J
AU  - Handley,W
AU  - Hansen,FK
AU  - Helou,G
AU  - Herranz,D
AU  - Hildebrandt,SR
AU  - Hivon,E
AU  - Huang,Z
AU  - Jaffe,AH
AU  - Jones,WC
AU  - Karakci,A
AU  - Keihanen,E
AU  - Keskitalo,R
AU  - Kiiveri,K
AU  - Kim,J
AU  - Kisner,TS
AU  - Knox,L
AU  - Krachmalnicoff,N
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lagache,G
AU  - Lamarre,J-M
AU  - Langer,M
AU  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Le,Jeune M
AU  - Leahy,JP
AU  - Lesgourgues,J
AU  - Levrier,F
AU  - Lewis,A
AU  - Liguori,M
AU  - Lilje,PB
AU  - Lilley,M
AU  - Lindholm,V
AU  - Lopez-Caniego,M
AU  - Lubin,PM
AU  - Ma,Y-Z
AU  - Macias-Perez,JF
AU  - Maggio,G
AU  - Maino,D
AU  - Mandolesi,N
AU  - Mangilli,A
AU  - Marcos-Caballero,A
AU  - Maris,M
AU  - Martin,PG
AU  - Martinelli,M
AU  - Martinez-Gonzalez,E
AU  - Matarrese,S
AU  - Mauri,N
AU  - McEwen,JD
AU  - Meerburg,PD
AU  - Meinhold,PR
AU  - Melchiorri,A
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Millea,M
AU  - Mitra,S
AU  - Miville-Deschenes,M-A
AU  - Molinari,D
AU  - Moneti,A
AU  - Montier,L
AU  - Morgante,G
AU  - Moss,A
AU  - Mottet,S
AU  - Munchmeyer,M
AU  - Natoli,P
AU  - Norgaard-Nielsen,HU
AU  - Oxborrow,CA
AU  - Pagano,L
AU  - Paoletti,D
AU  - Partridge,B
AU  - Patanchon,G
AU  - Pearson,TJ
AU  - Peel,M
AU  - Peiris,HV
AU  - Perrotta,F
AU  - Pettorino,V
AU  - Piacentini,F
AU  - Polastri,L
AU  - Polenta,G
AU  - Puget,J-L
AU  - Rachen,JP
AU  - Reinecke,M
AU  - Remazeilles,M
AU  - Renault,C
AU  - Renzi,A
AU  - Rocha,G
AU  - Rosset,C
AU  - Roudier,G
AU  - Rubino-Martin,JA
AU  - Ruiz-Granados,B
AU  - Salvati,L
AU  - Sandri,M
AU  - Savelainen,M
AU  - Scott
DO  - 0004-6361/201833880
PY  - 2020///
SN  - 0004-6361
TI  - Planck 2018 results: I. Overview and the cosmological legacy of Planck
T2  - Astronomy and Astrophysics: a European journal
UR  - http://dx.doi.org/10.1051/0004-6361/201833880
UR  - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000571763700001&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=a2bf6146997ec60c407a63945d4e92bb
UR  - https://www.aanda.org/articles/aa/full_html/2020/09/aa33880-18/aa33880-18.html
UR  - http://hdl.handle.net/10044/1/107607
VL  - 641
ER  -

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